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Exoplanet Biosignatures: Understanding Oxygen as a Biosignature in the Context of Its Environment

机译:系外行星的生物特征:在其环境中将氧气理解为生物特征

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摘要

We describe how environmental context can help determine whether oxygen (O-2) detected in extrasolar planetary observations is more likely to have a biological source. Here we provide an in-depth, interdisciplinary example of O-2 biosignature identification and observation, which serves as the prototype for the development of a general framework for biosignature assessment. Photosynthetically generated O-2 is a potentially strong biosignature, and at high abundance, it was originally thought to be an unambiguous indicator for life. However, as a biosignature, O-2 faces two major challenges: (1) it was only present at high abundance for a relatively short period of Earth's history and (2) we now know of several potential planetary mechanisms that can generate abundant O-2 without life being present. Consequently, our ability to interpret both the presence and absence of O-2 in an exoplanetary spectrum relies on understanding the environmental context. Here we examine the coevolution of life with the early Earth's environment to identify how the interplay of sources and sinks may have suppressed O-2 release into the atmosphere for several billion years, producing a false negative for biologically generated O-2. These studies suggest that planetary characteristics that may enhance false negatives should be considered when selecting targets for biosignature searches. We review the most recent knowledge of false positives for O-2, planetary processes that may generate abundant atmospheric O-2 without a biosphere. We provide examples of how future photometric, spectroscopic, and time-dependent observations of O-2 and other aspects of the planetary environment can be used to rule out false positives and thereby increase our confidence that any observed O-2 is indeed a biosignature. These insights will guide and inform the development of future exoplanet characterization missions. Key Words: BiosignaturesOxygenic photosynthesisExoplanetsPlanetary atmospheres. Astrobiology 18, xxx-xxx.
机译:我们描述了环境背景如何帮助确定在太阳系外行星观测中检测到的氧气(O-2)是否更可能具有生物来源。在这里,我们提供了O-2生物特征识别和观察的深入,跨学科的示例,作为开发生物特征评估通用框架的原型。光合作用产生的O-2是潜在的强大生物特征,并且在高丰度下,最初被认为是生命的明确指标。但是,作为生物签名,O-2面临两个主要挑战:(1)仅在地球历史上相对较短的时间内就以高丰度存在;(2)我们现在知道可以产生大量O-的几种潜在行星机制2没有生命存在。因此,我们解释系外光谱中O-2存在与否的能力取决于对环境的了解。在这里,我们研究了生命与地球早期环境的共同进化,以确定源和汇的相互作用如何抑制O-2向大气中释放数十亿年,从而对生物产生的O-2产生假阴性。这些研究表明,在选择生物特征搜索目标时应考虑可能会增加假阴性的行星特征。我们回顾了有关O-2假阳性的最新知识,O-2是可能在没有生物圈的情况下产生大量大气O-2的行星过程。我们提供了一些示例,说明如何使用O_2和行星环境其他方面的未来光度,光谱和时间相关观察来排除假阳性,从而增加我们对任何观察到的O-2确实是生物签名的信心。这些见解将指导并告知未来系外行星表征任务的发展。关键词:生物签名产氧光合作用系外行星行星大气。天体生物学18,xxx-xxx。

著录项

  • 来源
    《Astrobiology》 |2018年第6期|630-662|共33页
  • 作者单位

    Univ Washington, Dept Astron, POB 351580, Seattle, WA 98195 USA;

    Georgia Inst Technol, Sch Earth & Atmospher Sci, Atlanta, GA 30332 USA;

    NASA, Astrobiol Inst, Virtual Planetary Lab Team, Seattle, WA USA;

    NASA, Astrobiol Inst, Virtual Planetary Lab Team, Seattle, WA USA;

    NASA, Astrobiol Inst, Virtual Planetary Lab Team, Seattle, WA USA;

    NASA, Astrobiol Inst, Virtual Planetary Lab Team, Seattle, WA USA;

    Univ Washington, Dept Astron, POB 351580, Seattle, WA 98195 USA;

    NASA, Exoplanet Explorat Program, Jet Prop Lab, CALTECH, Pasadena, CA USA;

    German Aerosp Ctr, Inst Planetary Res Extrasolar Planets & Atmospher, Berlin, Germany;

    Univ Maryland, Sch Med, Dept Microbiol & Immunol, Baltimore, MD 21201 USA;

    Cornell Univ, Carl Sagan Inst, Ithaca, NY USA;

    Univ Tokyo, Dept Astron, Tokyo, Japan;

    Univ Washington, Dept Astron, POB 351580, Seattle, WA 98195 USA;

    Univ Washington, Dept Astron, POB 351580, Seattle, WA 98195 USA;

    NASA, Astrobiol Inst, Alternat Earths Team, Riverside, CA USA;

    NASA, Exoplanet Explorat Program, Jet Prop Lab, CALTECH, Pasadena, CA USA;

    German Aerosp Ctr, Inst Planetary Res Extrasolar Planets & Atmospher, Berlin, Germany;

  • 收录信息 美国《科学引文索引》(SCI);美国《化学文摘》(CA);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

  • 入库时间 2022-08-17 13:04:04

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